A newfound stellar remnant some 17,000 light-years away is not your everyday pulsar. For starters, the hyperdense, swiftly pirouetting object appears to belong to a rare class known as disrupted recycled pulsars. Pulsars are so known because they rotate rapidly—this one spins more than 40 times a second—and give off a beam of radio waves that sweeps across the sky, much like a lighthouse. To an outside observer the radiation appears to pulse each time the beam points in the observer’s direction.

A disrupted recycled pulsar is a former member of a binary stellar pairing that first exploded as a supernova and collapsed to an extraordinarily dense object known as a neutron star, before cannibalizing matter from its neighbor, spinning faster all the while, and finally breaking free from its binary companion when the neighbor exploded as a supernova itself. Disrupted recycled pulsars are uncommon—a recent study estimated that of more than 1,500 known pulsars, only eight are of the disrupted recycled variety.

That life history surely qualifies as interesting, but the most noteworthy aspect of the newly located pulsar, known as PSR J2007+2722, is the way it was discovered. The celestial rarity was located by the personal computers of individuals in the U.S. and Germany who had lent their idle processor time to [email protected], a campaign that has used hundreds of thousands of volunteered computers to mine astrophysical data sets for interesting phenomena. The discovery was announced in a paper published online in Science August 12.